Real-time wavefront control for the PALM-3000 high order adaptive optics system

We present a cost-effective scalable real-time wavefront control architecture based on off-the-shelf graphics processing units hosted in an ultra-low latency, high-bandwidth interconnect PC cluster environment composed of modules written in the component-oriented language of nesC. We demonstrate the architecture is capable of supporting the most computation and memory intensive wavefront reconstruction method (vector-matrix-multiply) at frame rates up to 2 KHz with latency under 250 &mgr;s for the PALM-3000 adaptive optics systems, a state-of-the-art upgrade on the 5.1 meter Hale Telescope that consists of a 64x64 subaperture Shack-Hartmann wavefront sensor and a 3368 active actuator high order deformable mirror in series with a 349 actuator "woofer" DM. This architecture can easily scale up to support larger AO systems at higher rates and lower latency.

[1]  Fang Shi,et al.  Real-time wavefront processors for the next generation of adaptive optics systems: a design and analysis , 2003, SPIE Astronomical Telescopes + Instrumentation.

[2]  Eric E. Bloemhof,et al.  Palomar adaptive optics project: status and performance , 2000, Astronomical Telescopes and Instrumentation.

[3]  David E. Culler,et al.  The nesC language: A holistic approach to networked embedded systems , 2003, PLDI '03.

[4]  Margo I. Seltzer,et al.  Berkeley DB , 1999, USENIX Annual Technical Conference, FREENIX Track.

[5]  Richard Dekany,et al.  PALM-3000: visible light AO on the 5.1-meter Telescope , 2006, SPIE Astronomical Telescopes + Instrumentation.

[6]  Philip Levis,et al.  TinyOS Programming: Introduction , 2009 .